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000850769 1001_ $$0P:(DE-HGF)0$$aHerrmann, V.$$b0$$eCorresponding author
000850769 245__ $$aProton-Proton- und Neutron-Proton-Bremsstrahlung im Potentialmodell
000850769 260__ $$aJülich$$bForschungszentrum Jülich GmbH Zentralbibliothek, Verlag$$c1993
000850769 300__ $$a144 p.
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000850769 4900_ $$aBerichte des Forschungszentrums Jülich$$v2840
000850769 520__ $$aThe nucleon-nucleon(NN) bremsstrahlung reaction is studied in the framework of a potential model. We investigate and explain the behavior of the most important corrections to the purely non-relativistic model considering only the external current; i. e. we include the relativistic spin correction, the one-body rescattering contribution and the Coulomb-effect, where it is needed. The important contribution of the two-body or meson-exchange current is treated in the soft-photon-approximation. In addition to the usual coplanar NN$_{\gamma}$ cross section we also study non-coplanar cross sections and spin observables like the analyzing power and spin correlation coefficients. It is shown that the behavior of the relativistic spin correction is governed by the $^{1}$S$_{0}$ partial-wave state, is almost energy independent and reduces the NN$_{\gamma}$ cross section by roughly 20 - 30%. The one-body rescattering contribution enhances the pp$\gamma$ cross section for the geometry of the last TRIUMF experiment by about 20% and thus almost compensates the effect of the relativistic spin corrections. The effects of each part of the NN interaction on the pp$\gamma$ observables is studied in the coplanar geometry. We find that these effects depend on the proton scatteringangles as well as on the considered observable. However, the tensor component of the NN interaction is important in all geometries. The comparison of different NN potential models yields that the NN$_{\gamma}$ reaction is not able to discriminate these potentials in their off-shell behavior, although the corresponding T-matrices deviate from each other off the energy shell. It is concluded that the occuring differences originate already from deviations on the energy shell or from the fact that the approximations made in the calculations for the two-body current are not of the same quality for all NN potential models.
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